2MASS J10220489+0200477 (Q77410656)

high proper-motion star

1 reference

1 reference

2MASS J10220489+0200477

1 reference

SDSS J102204.88+020047.5

catalog

Sloan Digital Sky Survey

1 reference

WISEA J102204.76+020043.4

1 reference

ULAS J102204.78+020043.9

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Gaia DR2 3856498658891737728

1 reference

0 references

−0.00001±0.00016

1 reference

distance from Earth

56.8 parsec

1 reference

Constraining the age-activity relation for cool stars: the Sloan Digital Sky Survey Data Release 5 low-mass star spectroscopic sample

34 parsec

1 reference

Meeting the cool neighbors. X. Ultracool dwarfs from the 2MASS all-sky data release

34±4 parsec

1 reference

The brown dwarf kinematics project I. Proper motions and tangential velocities for a large sample of late-type M, L, and T dwarfs

24.2±4.6 parsec

1 reference

Colors and kinematics of L dwarfs from the Sloan Digital Sky Survey

30.1823±0.3364 parsec

1 reference

parallax

33.132±0.3693 milliarcsecond

1 reference

0.0346±0.002 milliarcsecond

1 reference

The Hawaii infrared parallax program. II. Young ultracool field dwarfs

declination component of proper motion

−417.807±0.639 milliarcsecond per year

1 reference

−0.418±0.002 milliarcsecond per year

1 reference

The Hawaii infrared parallax program. II. Young ultracool field dwarfs

−429±7 milliarcsecond per year

1 reference

The Brown Dwarf Kinematics Project (BDKP). III. Parallaxes for 70 ultracool dwarfs

−398±16 milliarcsecond per year

2 references

Colors and kinematics of L dwarfs from the Sloan Digital Sky Survey

Proper motions of field L and T dwarfs

−394±18 milliarcsecond per year

1 reference

The brown dwarf kinematics project I. Proper motions and tangential velocities for a large sample of late-type M, L, and T dwarfs

right ascension component of proper motion

−179.65±0.59 milliarcsecond per year

1 reference

−0.178±0.002 milliarcsecond per year

1 reference

The Hawaii infrared parallax program. II. Young ultracool field dwarfs

−156±7 milliarcsecond per year

1 reference

The Brown Dwarf Kinematics Project (BDKP). III. Parallaxes for 70 ultracool dwarfs

−173±18 milliarcsecond per year

2 references

Colors and kinematics of L dwarfs from the Sloan Digital Sky Survey

Proper motions of field L and T dwarfs

−178±18 milliarcsecond per year

1 reference

The brown dwarf kinematics project I. Proper motions and tangential velocities for a large sample of late-type M, L, and T dwarfs

radial velocity

−3±0 kilometre per second

1 reference

−1.4±18.7 kilometre per second

1 reference

Colors and kinematics of L dwarfs from the Sloan Digital Sky Survey

spectral class

M9.0V

1 reference

SpeX SPECTROSCOPY OF UNRESOLVED VERY LOW MASS BINARIES. II. IDENTIFICATION OF 14 CANDIDATE BINARIES WITH LATE-M/EARLY-L AND T DWARF COMPONENTS

L0pec?

1 reference

A Sample of Very Young Field L Dwarfs and Implications for the Brown Dwarf “Lithium Test” at Early Ages

L0

1 reference

Colors and kinematics of L dwarfs from the Sloan Digital Sky Survey

L0e

1 reference

Constraining the age-activity relation for cool stars: the Sloan Digital Sky Survey Data Release 5 low-mass star spectroscopic sample

(M9)

1 reference

Meeting the cool neighbors. X. Ultracool dwarfs from the 2MASS all-sky data release

24.426±1.082

1 reference

The Fifth Data Release of the Sloan Digital Sky Survey

22.855±0.174

g' band

1 reference

The Fifth Data Release of the Sloan Digital Sky Survey

20.802±0.052

r' band

1 reference

The Fifth Data Release of the Sloan Digital Sky Survey

14.05±0.01

J band

1 reference

Photometric brown-dwarf classification. II. A homogeneous sample of 1361 L and T dwarfs brighter than J = 17.5 with accurate spectral types

18.323±0.01

i' band

1 reference

16.481±0.009

z' band

1 reference

13.44±0.01

H band

1 reference

Photometric brown-dwarf classification. II. A homogeneous sample of 1361 L and T dwarfs brighter than J = 17.5 with accurate spectral types

12.9±0.01

K band

1 reference

Photometric brown-dwarf classification. II. A homogeneous sample of 1361 L and T dwarfs brighter than J = 17.5 with accurate spectral types

18.7918±0.0044

1 reference

1 reference

155.52037356122090 degree

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declination

2.01327996696070 degree

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